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Table 4.

Number of joint detections by Rubin operating in synergy with ET triangular shape operating as a single observatory, and as part of a global network of GW detectors (indicated in the second column from the left).

APR4 BLh

Ω90 Transient Uniform Gaussian Uniform Gaussian
[deg2] Followed Detected Followed Detected Followed Detected Followed Detected
1ep/2ep 1ep/2ep 1ep/2ep 1ep/2ep
α = 0.5 ET-Δ 100 KN 168 (2.1%) 72/47 144 (1.8%) 76/57 172 (2.2%) 64/49 144 (1.9%) 100/79
KN+GRB 82/59 86/70 77/62 108/91

ET-Δ
+
LVKI
20 KN 1043 (3.5%) 383/228 655 (2.2%) 326/204 956 (3.2%) 313/188 646 (2.2%) 444/296
KN+GRB 447/279 366/246 378/237 469/337

ET-Δ
+
1CE
10 KN 2097 (4.4%) 546/285 1242 (2.6%) 470/252 1930 (4.0%) 445/241 1227 (2.6%) 673/380
KN+GRB 680/381 552/327 579/328 747/456

ET-Δ
+
2CE
5 KN 13435 (26.6%) 978/442 10033 (19.9%) 900/387 12701 (25.2%) 812/368 9671 (19.2%) 1408/613
KN+GRB 1358/628 1238/564 1186/541 1744/799

α = 1.0 ET-Δ 100 KN 846 (10.2%) 346/251 695 (8.4%) 392/277 825 (10.0%) 337/246 695 (8.4%) 475/381
KN+GRB 383/282 416/301 379/273 497/403

ET-Δ
+
LVKI
20 KN 5231 (17.4%) 1896/1148 3287 (10.9%) 1740/1132 4825 (16.0%) 1566/971 3224 (10.7%) 2248/1545
KN+GRB 2108/1306 1859/1229 1787/1127 2335/1646

ET-Δ
+
1CE
10 KN 10188 (21.4%) 2772/1533 6072 (12.7%) 2505/1436 9320 (19.5%) 2269/1263 6002 (12.6%) 3496/2023
KN+GRB 3201/1806 2793/1654 2702/1538 3726/2255

ET-Δ
+
2CE
5 KN 67949 (134.8%) 5102/2276 50440 (100%) 4666/2147 64113 (127.2%) 4290/1911 48557 (96.3%) 7301/3276
KN+GRB 6356/2827 5828/2680 5548/2473 8423/3857

Notes. The table reports the numbers of GW events detected with a sky localisation smaller than the threshold, Ω90, and within Rubin's footprint. These events are the ones followed up by Rubin and indicated as followed in Columns 5, 7, 9 and 11. The percentage of Rubin's observational time required to follow up all of them is given in parentheses. The corresponding numbers of KN and KN+GRB detections are given in Columns 6, 8, 10, and 12 and indicated with detected both for the 1ep and 2ep detection strategies. The table lists the results for the APR4 and BLh EOSs, the uniform and Gaussian NS mass distributions both for the fiducial (α = 1.0) and pessimistic (α = 0.5) populations. All listed numbers refer to 10 years of observations and include the duty cycle for the GW detectors and Rubin as described in the text.

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